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A plasmoid-model for mass loss from stars on the upper red giant branch: The mass loss rate is controlled by the number of density scale heights in the convection zone

Fuente: arXiv

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Bibliographic Details
Main Authors:	MacDonald, J., Mullan, D. J.
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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